Olivier S. Barnouin

TL;DR: In this paper, an analysis of Lutetia's surface lineaments was performed using the OSIRIS camera, and the results indicated that the orientation of lineaments could be explained by three impact craters: the Massilia and the NPCC craters observed in the northern hemisphere, and candidate crater Suspicio inferred to be in the southern hemisphere.

TL;DR: In this article, the authors used a radar-derived shape model for the asteroid, along with current best estimates for the orbital solution of Apophis to simulate the encounter trajectory, and performed a large parameter sweep over different potential encounter orientations and bulk densities for the body.

TL;DR: In this paper, the authors analyzed over 100 martian gully sites using orbital data collected by the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) and High Resolution Imaging Science Experiment (HiRISE) on the Mars Reconnaissance Orbiter (MRO).

TL;DR: In this paper, a shape model derived from stereophotoclinometric analysis was used to constrain the mode of pond formation from three existing models, and the locations of 55 pond candidates identified in images registered to the new shape model were updated.

TL;DR: In this paper, the authors present results from numerical simulations of the DART impact using the CTH shock physics code with 2D homogenous asteroid models, which greatly reduces the parameter space required for more expensive 3D simulations.